فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri - Paris Observatory

A process based on the effects of → opacity (κ) that drives the
→ pulsations
of many types of variable stars. Consider a layer of material within a
star and suppose that it undergoes inward contraction. This inward
motion tends to compress the layer and increase the density. Therefore
the layer becomes more opaque (See also → partial ionization zone).
If a certain amount of flux comes from
the deeper layers it gets stuck in the high κ region. The energy
accumulates and heat builds up beneath it. The pressure rises below
the layer, pushing it outward. The layer expands as it moves
outward, cools and becomes more transparent to radiation. Energy can
now escape from below the layer, and pressure beneath the layer
diminishes. The layer falls inward and the cycle repeats. The
κ mechanism is believed to account for the pulsations of several
star families, including → Delta Scuti stars,
→ Beta Cephei variables, → Cepheids,
and → RR Lyrae stars
(See Baker & Kippenhahn, 1962, Zeitschrift für Astrophysik 54, 114). Same as
κ effect and → valve mechanism.
See also → gamma mechanism.